Fig. 5.
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Top panels: Dense Basis SFHs based on the LRD1 (left) and LRD2 (right) PSF photometry. Solid lines show the 50th percentile and shaded regions the 16th-84th percentiles, color-coded by redshift. The thicker line depicts the low-z case, which corresponds to the photo-z of the galaxy group. Middle panels: Dense Basis SFHs derived from the stellar component only (obtained by subtracting the AGN photometry from the PSF photometry; Sect. 4.3), color-coded by redshift. The inset in the left panel shows a zoomed-in view of the LRD1 mid-z SFH. Bottom panels (from left to right): SFHs derived for SAT0, SAT1, and SAT2, color-coded by redshift.
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